Saturday, April 2, 2016
Live Jupiter special! It was a beautiful night in Melbourne, then about 10:30 just half an hour before "go-live" the clouds came from nowhere. Fortunately they didn't hang around for long - it must have been a moment of climatological rebellion with the impending ending of daylight saving several hours later. It was a little bit sad that the Great Red Spot had already transited before we got to air - but I did get some great footage of it before the clouds swept in. By the time we were on air the clouds had cleared and we continued on with the "boring side of Jupiter". I have been in a number of virtual events usually with my DSLR plugged directly into the laptop and screen sharing the Cannon EOS utility and using live view. The best method of course is a astronomy camera in a web cam setup. On this occasion I tried something a little different. Using the iPhone 6 and an eyepiece adapter, a 25mm eyepiece and the 645 App I was able to take some of the light of Jupiter out (its usually too bright to see any detail on the disk) by taking the ISO to 32 and setting the exposure time to 1/100 of a sec and the through the lens view adjusts to a "what you see is what you get" view. Then sharing that back to my MacBook using reflection, I was able to then screen share the Reflection App into the Google Plus Hangout. Pretty cool! 14inch Smart Dobbie>Barlow>25mm Plossl Eyepiece>Smart Phone Telescope Adapter>645 Pro [Application]>ISO 32 & 1/100 Settings>Reflector to MacBookAir>Reflector Screen record. An excellent result, but more essentially here, what astronomy can we do with using equipment that we already have or that's relatively inexpensive, but easily accessible. Thanks to the Global Star Party for hosting me on the show!
Monday, March 14, 2016
Friday, March 4, 2016
OBS P. B. Lake
PK16B14A C2016 03 03.43620 05 51 24.42 -34 16 10.7 18.4 N Q62
PK16B14A C2016 03 03.43801 05 51 24.54 -34 16 08.7 18.3 N Q62
PK16B14A C2016 03 03.43976 05 51 24.62 -34 16 06.7 18.5 N Q62
PK16B14A C2016 03 03.44150 05 51 24.72 -34 16 04.9 18.4 N Q62
PK16B14A C2016 03 03.44324 05 51 24.83 -34 16 02.8 18.2 N Q62
PK16B14A C2016 03 03.44498 05 51 24.95 -34 16 01.1 18.3 N Q62
PK16B14A C2016 03 03.44672 05 51 25.05 -34 15 58.9 18.2 N Q62
PK16B14A C2016 03 03.44860 05 51 25.15 -34 15 56.9 18.3 N Q62
PK16B14A C2016 03 03.45035 05 51 25.26 -34 15 55.1 18.3 N Q62
PK16B14A C2016 03 03.45209 05 51 25.35 -34 15 53.2 18.2 N Q62
PK16B14A C2016 03 03.45383 05 51 25.47 -34 15 51.0 18.3 N Q62
PK16B14A C2016 03 03.45557 05 51 25.57 -34 15 49.2 18.4 N Q62
Looking forward to a nice telescopic show late in the month whilst we are at NACAA.
Sunday, February 14, 2016
Thursday, February 11, 2016
UPDATE: Feb 27th 2016 I have got them calibrated now. The iPhone6 version calibration is still a bit rough. Lining up on the Helium Lines seems to produce the best results. The camera response is markedly different for the iPhone over the Cannon 550D. Now that I know what we are looking at here, next time I image I can make sure I get the image in a bit better focus. I have also found a way to reduce camera shake by delaying the shutter open until 3 secs after you press the shutter button. Whilst you can see visually the same lines, when extracted using Visual Spec the camera response seems a bit different. Astronomical Spectroscopy for Amateurs. It is well written but looks quite daunting when you first pick it up. However if you work through it bit by bit, its a great book with everything you need to know. Feeling a little more confident, I invested in the next logical step - a Star Analyser 100. This is the entry level standard for beginners, and produces fine results as we'll see. After passing it around the family to have a look at the cool effects looking at the ceiling lights, I lost the plot and departed from Ken's careful, meticulously presented steps, with the outrageous thought - I wonder how this baby would go on an iPhone! I am constantly amazing at STEM events and star parties how the "younglings" immediately are so amazed by what they see through the eyepiece they want to whip out the smartphone and take an image home with them. Surely it couldn't possibly work. After all the iPhone 6 sensor is only 4.8mm by 3.6mm, it has a focal length of 29mm and is f2.2. But its an 8M pixel camera (said my evil twin subconscious), your Fingerlakes PL11000M is only 11M pixels so its only 3000 less pixels, how bad could it be....hang-on whats the pixel size ...ah 1.5um versus 9um, interesting. So the sensor is 3264 x 2448, interesting ..... iPhones do take good photos......on a sunny day.....not in the night sky. This went on for a while! So in the end there was nothing else to do but try it, and learn from your spectacular mistakes! 645 Pro could even do it with an Kodak Ektrachrome 64 film "feel to it". NOTE: to those born after the 90's, can you imagine only getting 36 images on one roll of film and not being able "to delete the bad ones" until after you had paid $25 and sent it off to the developers and had it returned to your letter box. In those days the lens ONLY pointed away from you - THE HORROR! Anyway I digress. 645 Pro basically turns your iPhone into a simulated DSLR and enters the workflow of the photography before any JPEG compression. You can set ISO and shutter speed, bracket exposures do all sorts of things that you can do on a DSLR. With my trusty new app, my camera adapter, my star analyser, a 25mm eyepiece, I was ready for action.
Friday, February 5, 2016
In my continuing efforts to de-mystify the art of Asteroid Astrometry, I thought I'd follow up last week's article on about 2016 BE with a deeper examination of the Uncertainty parameter when its listed in orbital elements. This week there is some attention on 2013 TX68 which will possibly make a record close pass of 11,000 klms or possibly be 40 times further away than the moon on March the 5th. I can see that puzzled look on your face ;-) 2013 TX68 is also a Virtual Impactor in 2017, a term we discussed last week. So firstly lets get some perspective on this uncertainty thing. 2011 CF66 was also listed as a virtual impactor for Feb 2nd 2016, it didn't hit us, no-one was worried if it would, and in fact no-one has any idea where it actually is. It is only a tiny asteroid about 3-9m in diameter and wouldn't have done any damage even if it did. In fact there are 20 other virtual impactors listed in the Risk Table this year, the next one might approach on Feb 18th, is 2009 VZ39, and is slightly smaller than 2013 TX68. 2009 VZ39 is also in the daytime sky and not observable for follow up and further confirmation. I only highlight this to emphasise the point here - all asteroids once they are discovered need to be tracked for sometime, to improve the precision of the orbit before any pronouncements about where they are going to be at a certain point in time. The difference between 2013 TX68 and 2009 VZ39 for example is that 2013 TX68 was observed for 31 data positions (astrometry) over 3 nights where as 2009 VZ39 was observed on only one night with 8 astrometric data positions. If you look at the orbital elements for 2013 TX68 the uncertainty parameter is listed as 7, where as for 2009 VZ39 there is not even enough data to start that calculation. For 2011 CF66, there is a 1.1e-8 chance of a collision between 2016 and 2114, so its mathematically possible, but highly unlikely. NASA/JPL produced this nice graph with it's press release this week which illustrates the point well.
Friday, January 29, 2016
Sentry Risk Table is for the 3rd February 2053 .... NOT ON THIS PASS!!!! As you would expect the "zone of uncertainty" for 2053 is much large than the "zone of uncertainty" for next week. So it will take many further observations before it is (most likely) removed from the risk table. Its current risk table score of Torino-0 just means that at this point the chance of a collision in 2053 has not been able to be eliminated at this stage. Measured position: K16B00E KC2016 01 28.46044 12 04 01.15 +65 50 49.0 16.9 R H06 K16B00E KC2016 01 28.46319 12 04 09.44 +65 49 54.8 17.3 R H06 K16B00E KC2016 01 28.46604 12 04 18.01 +65 48 58.7 17.4 R H06